MgH lines in the spectrum of Arcturus

dc.contributor.author	Kushniruk, I.O.
dc.contributor.author	Pavlenko, Ya.V.
dc.contributor.author	Kaminskiy, B.M.
dc.date.accessioned	2017-06-06T19:04:32Z
dc.date.available	2017-06-06T19:04:32Z
dc.date.issued	2013
dc.identifier.citation	MgH lines in the spectrum of Arcturus / I.O. Kushniruk, Ya.V. Pavlenko, B.M. Kaminskiy // Advances in Astronomy and Space Physics. — 2013. — Т. 3., вип. 1. — С. 29-31. — Бібліогр.: 12 назв. — англ.	uk_UA
dc.identifier.issn	2227-1481
dc.identifier.uri	http://dspace.nbuv.gov.ua/handle/123456789/119418
dc.description.abstract	The synthetic spectra of MgH lines were computed for the grid of the model atmospheres and compared with the observed spectrum of Arcturus. The parameters of the atmosphere of Arcturus for log g = 1.5 and Tₑff = 4300K were via minimization of deviation between observed and computed spectra and compared with the results of other studies.	uk_UA
dc.description.sponsorship	We thank to Profs. Hinkle, Kurucz, and VALD team for providing databases of astrophysical data used in our work, Oleksiy Ivanyuk and Larisa Yakovina for the helpful comments, and anonymous Referee for some positive remarks.	uk_UA
dc.language.iso	en	uk_UA
dc.publisher	Головна астрономічна обсерваторія НАН України	uk_UA
dc.relation.ispartof	Advances in Astronomy and Space Physics
dc.title	MgH lines in the spectrum of Arcturus	uk_UA
dc.type	Article	uk_UA
dc.status	published earlier	uk_UA